Title of article
The CO2 gas Cherenkov detectors for the Jefferson Lab Hall-A spectrometers
Author/Authors
Iodice، نويسنده , , M. and Cisbani، نويسنده , , E. and Colilli، نويسنده , , S. and Crateri، نويسنده , , R. and Frullani، نويسنده , , S. and Garibaldi، نويسنده , , F. and Giuliani، نويسنده , , F. and Gricia، نويسنده , , M. and Lucentini، نويسنده , , M. and Mostarda، نويسنده , , A. and Pierangeli، نويسنده , , L. and Santavenere، نويسنده , , F. and Urciuoli، نويسنده , , G.M. and De Leo، نويسنده , , R. and Lagamba، نويسنده , , Zakary L. and Leone، نويسنده , , A. and Perrino، نويسنده , , R. and Kerhoas، نويسنده , , S. and Lugol، نويسنده , , I.C. and Mazeav، نويسنده , , B. and Vernin، نويسنده , , P. and Zaccarian، نويسنده , , A.، نويسنده ,
Pages
15
From page
223
To page
237
Abstract
Two threshold gas Cherenkov counters have been constructed for the electron and hadron High Resolution Spectrometers (HRS) of the Jefferson Lab Experimental Hall-A. These counters are intended to separate electrons/positrons from other particles up to 4 GeVc. The counters are operated at atmospheric pressure with CO2. Each counter is equipped with ten mirrors. Light weight, thin spherical mirrors (∼ 5.5 × 10−3 radiation lengths) have been employed resulting in a total thickness of ∼ 1.4 × 10−2 radiation lengths crossed by the particles. A prototype of the counter has been tested at CERN with a mixed beam of positrons, pions and protons from 1 to 4 GeVc. Its detection efficiency for positrons and the rejection ratios for pions and protons have been measured as a function of the pulse height response (or equivalently the number of photoelectrons). An improvement of 34% in the number of photoelectrons has been obtained by using a wavelength shifter coated on the photocathode glass window. With such an improvement in 1 m long radiator, an inefficiency for positrons less than 10−3 and rejection ratios πe at the level of few 10−3 and pe smaller than 10−3 have been obtained for pulse heights above 2 photoelectrons. Contaminations of particles below the Cherenkov threshold is fully understood considering δ-rays production.
Journal title
Astroparticle Physics
Record number
2005508
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